Photometric and spectroscopic evolution of the interacting transient at 2016jbu(Gaia16cfr)

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dc.contributor.authorBrennan, S.J.
dc.contributor.authorFraser, M.
dc.contributor.authorJohansson, J.
dc.contributor.authorPastorello, A.
dc.contributor.authorKotak, R.
dc.contributor.authorStevance, H.F.
dc.contributor.authorChen, T.-W.
dc.contributor.authorEldridge, J.J.
dc.contributor.authorBose, S.
dc.contributor.authorBrown, P.J.
dc.contributor.authorCallis, E.
dc.contributor.authorCartier, R.
dc.contributor.authorDennefeld, M.
dc.contributor.authorDong, Subo
dc.contributor.authorDuffy, P.
dc.contributor.authorElias Rosa, N.
dc.contributor.authorHosseinzadeh, G.
dc.contributor.authorHsiao, E.
dc.contributor.authorKuncarayakti, H.
dc.contributor.authorMartin Carrillo, A.
dc.contributor.authorMonard, B.
dc.contributor.authorNyholm, A.
dc.contributor.authorPignata, G.
dc.contributor.authorSand, D.
dc.contributor.authorShappee, B.J.
dc.contributor.authorSmartt, S.J.
dc.contributor.authorTucker, B.E.
dc.contributor.authorWyrzykowski, L.
dc.contributor.authorAbbot, H.
dc.contributor.authorBenetti, S.
dc.contributor.authorBento, J.
dc.contributor.authorBlondin, S.
dc.contributor.authorChen, Ping
dc.contributor.authorDelgado, A.
dc.contributor.authorGalbany, L.
dc.contributor.authorGromadzki, M.
dc.contributor.authorGutierrez, C.P.
dc.contributor.authorHanlon, L.
dc.contributor.authorHarrison, D.L.
dc.contributor.authorHiramatsu, D.
dc.contributor.authorHodgkin, S.T.
dc.contributor.authorHoloien, T.W.-S.
dc.contributor.authorHowell, D.A.
dc.contributor.authorInserra, C.
dc.contributor.authorKankare, E.
dc.contributor.authorKozłowski, S.
dc.contributor.authorMüller Bravo, T.E.
dc.contributor.authorMaguire, K.
dc.contributor.authorMcCully, C.
dc.contributor.authorMeintjes, P.
dc.contributor.authorMorrell, N.
dc.contributor.authorNicholl, M.
dc.contributor.authorO'Neill, D.
dc.contributor.authorPietrukowicz, P.
dc.contributor.authorPoleski, R.
dc.contributor.authorPrieto, J.L.
dc.contributor.authorRau, A.
dc.contributor.authorReichart, D.E.
dc.contributor.authorSchweyer, T.
dc.contributor.authorShahbandeh, M.
dc.contributor.authorSkowron, J.
dc.contributor.authorSollerman, J.
dc.contributor.authorSoszyński, I.
dc.contributor.authorStritzinger, M.D.
dc.contributor.authorSzymański, M.
dc.contributor.authorTartaglia, L.
dc.contributor.authorUdalski, A.
dc.contributor.authorUlaczyk, K.
dc.contributor.authorYoung, D.R.
dc.contributor.authorVan Leeuwen, M.
dc.contributor.authorVan Soelen, B.
dc.date.accessioned2023-11-28T13:47:17Z
dc.date.available2023-11-28T13:47:17Z
dc.date.issued2022-07-01
dc.descriptionIndexación: Scopus.es
dc.description.abstractWe present the results from a high-cadence, multiwavelength observation campaign of AT 2016jbu (aka Gaia16cfr), an interacting transient. This data set complements the current literature by adding higher cadence as well as extended coverage of the light-curve evolution and late-time spectroscopic evolution. Photometric coverage reveals that AT 2016jbu underwent significant photometric variability followed by two luminous events, the latter of which reached an absolute magnitude of MV ∼-18.5 mag. This is similar to the transient SN 2009ip whose nature is still debated. Spectra are dominated by narrow emission lines and show a blue continuum during the peak of the second event. AT 2016jbu shows signatures of a complex, non-homogeneous circumstellar material (CSM). We see slowly evolving asymmetric hydrogen line profiles, with velocities of 500 km s-1 seen in narrow emission features from a slow-moving CSM, and up to 10 000 km s-1 seen in broad absorption from some high-velocity material. Late-time spectra (∼+1 yr) show a lack of forbidden emission lines expected from a core-collapse supernova and are dominated by strong emission from H, He i, and Ca ii. Strong asymmetric emission features, a bumpy light curve, and continually evolving spectra suggest an inhibit nebular phase. We compare the evolution of H α among SN 2009ip-like transients and find possible evidence for orientation angle effects. The light-curve evolution of AT 2016jbu suggests similar, but not identical, circumstellar environments to other SN 2009ip-like transients. © 2022 The Author(s) Published by Oxford University Press on behalf of Royal Astronomical Society.es
dc.description.urihttps://academic-oup-com.recursosbiblioteca.unab.cl/mnras/article/513/4/5642/6581585
dc.identifier.citationMonthly Notices of the Royal Astronomical Society, Volume 513, Issue 4, Pages 5642 - 5665,July 2022es
dc.identifier.doi10.1093/mnras/stac1243
dc.identifier.issn0035-8711
dc.identifier.urihttps://repositorio.unab.cl/xmlui/handle/ria/54195
dc.language.isoenes
dc.publisherOxford University Presses
dc.rights.licenseCC BY 4.0 DEED Atribución 4.0 Internacional
dc.rights.urihttps://creativecommons.org/licenses/by/4.0/deed.es
dc.subjectCircumstellar matteres
dc.subjectStars: Massivees
dc.subjectSupernovae: Individual: AT 2016jbues
dc.subjectGaia16cfres
dc.subjectSN 2009ipes
dc.titlePhotometric and spectroscopic evolution of the interacting transient at 2016jbu(Gaia16cfr)es
dc.typeArtículoes
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